Author/Authors :
Nishiuchi، نويسنده , , M and Koyama، نويسنده , , K and Awaki، نويسنده , , H and Tsuru، نويسنده , , T and Sakano، نويسنده , , M and Hamaguchi، نويسنده , , K and Murakami، نويسنده , , H and Tsunemi، نويسنده , , H and Hayashida، نويسنده , , K and Kitamoto، نويسنده , , S and Miyata، نويسنده , , E and Dotani، نويسنده , , T and Ozaki، نويسنده , , M and Bautz، نويسنده , , M and Doty، نويسنده , , J and Kissel، نويسنده , , S and Foster، نويسنده , , R and Ricker، نويسنده , , G، نويسنده ,
Abstract :
We report on the hard X-ray response of the CCD detector for the X-ray imaging spectrometer (XIS), to be launched on the next Japanese X-ray Astronomical Satellite, ASTRO-E, in February 2000. XIS is prepared by an international team, comprised of MIT (USA), ISAS, Osaka University and Kyoto University (JAPAN). We have evaluated the X-ray response of the XIS in its high-energy band (1.5–10 keV). Data from the fluorescent line emission of Al, Cl, Ti, Ni, Fe, Zn, Se were used to construct the response function of the CCD detectors. Details of the response function – including the energy-scale, linearity, energy resolution, quantum efficiency –, are given as a function of incident X-ray energy. We find that the tail component of high-energy photopeaks are produced by events with incomplete charge collection. We also conclude that the size of the charge clouds can be estimated using the shapes of the tail components.
